FSR 1352

(MWSC 1334)

Click to load Aladin Lite
0.86 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 171
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
FSR 1352 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for FSR 1352 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 116.573 -34.31 0.262 -2.066 3.139 –
Almeida et al. 2025 116.613 -34.295 – – – –
Hunt & Reffert 2024 116.602 -34.291 0.268 -2.104 3.106 –
Celli et al. 2024 116.614 -34.287 – – – –
Cavallo et al. 2024 116.503 -34.319 0.269 – – –
Hunt & Reffert 2023 116.602 -34.291 0.268 -2.104 3.106 –
Just et al. 2023 116.613 -34.278 – – – –
Dias et al. 2021 116.613 -34.295 0.234 -1.997 3.158 –
Cantat-Gaudin et al. 2020 116.614 -34.287 0.24 -1.981 3.148 –
Cantat-Gaudin & Anders 2020 116.614 -34.287 0.24 -1.981 3.148 –
Cantat-Gaudin et al. 2018 116.614 -34.287 0.24 -1.981 3.148 –
Kharchenko et al. 2016 116.613 -34.278 – – – –
Kharchenko et al. 2013 116.617 -34.28 – -3.86 5.62 –
Froebrich et al. 2007 116.6 -34.301 – – – –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Almeida et al. 2025 3.40 2.70 – 5 – 268 – –
Hunt & Reffert 2024 – – – – – 2784* – –
Celli et al. 2024 – – – 4 – 146 – –
Cavallo et al. 2024 4.07 3.03 – 19 0.800 – – –
Hunt & Reffert 2023 3.33 3.24 2.66 8 – – – –
Just et al. 2023 – – – 191 – 44 – –
Dias et al. 2021 3.40 2.70 – 5 -0.097 – – –
Cantat-Gaudin et al. 2020 3.65 2.57 – 3 – – – –
Cantat-Gaudin & Anders 2020 3.72 – – – – – – –
Cantat-Gaudin et al. 2018 3.72 – – – – – – –
Kharchenko et al. 2016 1.51 2.00 – 191 – – – –
Kharchenko et al. 2013 1.51 2.00 – 191 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 1351 52.0 116.48 -34.34 0.27 -2.09 3.15 – 0.65
Cmg 1066 50.3 116.57 -34.31 0.27 -2.06 3.17 – 0.0

💡 Note: The % column shows the percentage of members that FSR 1352 shares with each listed object.

Visualization
ℹī¸
FSR 1352 UCC
FSR 1352 HUNT23
FSR 1352 CANTAT20
Galactocentric position diagram